A twin cluster to Collinder 69 in the lambda Orionis star forming region ?

Details A twin cluster to Collinder 69 in the lambda Orionis star forming region ? A twin cluster to Collinder 69 in the lambda Orionis star forming region ?

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008xmm..prop...56s&link_type=abstract

XMM-Newton Proposal ID #06021201

Other

Stars, White Dwarfs, Solar System, Lambdaori - F1

Scientific paper

The lambda Ori star forming region (5 Myr, 400 pc) is surrounded by a 5 x 5 deg wide molecular ring probably formed by a supernova explosion. Our previous multi-wavelength studies focused on the most well-known areas within the cloud complex. For a complete picture of star formation, believed to be determined by the supernova blast, the large-scale distribution of the pre-main sequence population in lambda Ori needs to be examined. We suspect a further pre-main sequence cluster to be associated with a concentration of B-type stars near the NE of the molecular ring. A search for X-ray emission is the most efficient way of identifying the low-mass cluster. The properties of its members will then be compared to the other lambda Ori subgroups.

Affiliated with

Also associated with

No associations

Rating

A twin cluster to Collinder 69 in the lambda Orionis star forming region ? does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with A twin cluster to Collinder 69 in the lambda Orionis star forming region ?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A twin cluster to Collinder 69 in the lambda Orionis star forming region ? will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-866140